Results 111 to 120 of about 4,621,719 (221)

Exploring the link between molecular cloud ices and chondritic organic matter in laboratory. [PDF]

Nat Commun, 2021
Danger G, Vinogradoff V, Matzka M, Viennet JC, Remusat L, Bernard S, Ruf A, Le Sergeant d'Hendecourt L, Schmitt-Kopplin P.   +8 more
europepmc   +1 more source

Global Collapses and Expansions in Star-Forming Clouds

, 2009
Spectral molecular line profile observations of star-forming molecular clouds sometimes show distinct red asymmetric double-peaked molecular line profiles with weaker blue peaks and stronger red peaks.
Adams, Adelson, Aguti, Arons, Belloche, Bernes, Bian, Carolan, Di Francesco, Evans, Fiege, Fiege, Fuller, Gao, Hammersley, Harvey, Hennebelle, Hogerheijde, Hu, Jørgensen, Kenyon, Keto, Lada, Larson, Lee, Lou, Lou, Lou, Lou, MacLow, Mardones, Matthews, Matzner, Matzner, McKee, Moraghan, Moriarty-Schieven, Myers, Myers, Nakano, Ossenkopf, Ostriker, Park, Park, Park, Rawlings, Redman, Redman, Saito, Schöier, Shang, Shen, Shirley, Shreider, Shu, Shu, Shu, Shu, Su, Tafalla, Tafalla, Tafalla, Thompson, Tsamis, van der Tak, Van Zadelhoff, Velusamy, Wang, Ward-Thompson, Wilner, Wu, Yang Gao, Yu, Yu, Yu-Qing Lou, Zhou, Zhou, Zweibel   +77 more
core   +1 more source

Detection of submillimeter /870-micron/ CO emission from the Orion molecular cloud [PDF]

, 1977
T. G. Phillips, G. Neugebauer, M. W. Werner, P. J. Huggins   +3 more
openalex   +1 more source

Jets in Molecular Clouds [PDF]

Symposium - International Astronomical Union, 1984
There is now growing evidence that the cosmic jet phenomenon manifests itself in a remarkable way in regions of active star formation embedded in dense molecular clouds. The first indications for oppositely directed, supersonic outflows from young stars were provided by molecular line observations (most notably of CO) which detected spatially separated
openaire   +1 more source

Star Formation in Clouds of Molecular Hydrogen [PDF]

, 1975
V. C. Reddish
openalex   +1 more source

CO observations of spiral structure and the lifetime of giant molecular clouds [PDF]

, 1979
N. Z. Scoville, P. M. Solomon, D. B. Sanders   +2 more
openalex   +1 more source

Reviewing Molecular Clouds

, 2017
The star formation process involves a wide range of spatial scales, densities and temperatures. Herschel observations of the cold and low density molecular gas extending tens of parsecs, that constitutes the bulk of the molecular clouds of the Milky Way, have shown a network of dense structures in the shape of filaments.
openaire   +2 more sources

Theoretical studies of interstellar molecular shocks - IV. The sulphur chemistry in diffuse clouds [PDF]

, 1986
G. Pineau des Forêts, E. Roueff, D. R. Flower   +2 more
openalex   +1 more source

Ice in the Taurus molecular cloud: modelling of the 3- m profile [PDF]

, 1985
C. E. P. M. van de Bult, J. Mayo Greenberg, D. C. B. Whittet   +2 more
openalex   +1 more source

Potassium isotope anomalies in meteorites inherited from the protosolar molecular cloud. [PDF]

Sci Adv, 2020
Ku Y, Jacobsen SB.
europepmc   +1 more source